Talk:Pair production

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Can we please remove this formula?[edit]

After reading this page, I could not possibly imagine this formula being useful to any reader, so I decided to go to the source ("Koehn, C., Ebert, U., Angular distribution of Bremsstrahlung photons and of positrons for calculations of terrestrial gamma-ray flashes and positron beams, Atmos. Res. (2014), vol. 135-136, pp. 432-465"). I assumed there would be no way someone could even correctly copy this formula into the page. I made it as far as I2 where there is a sign error in wikipedia compared to the paper. This clearly does not belong in the page, and should be removed, since anyone remotely interested in the equation would simply refer to the paper. Unfortunately, I believe this requires a rather substantial rewrite. — Preceding unsigned comment added by 129.67.38.58 (talk) 19:44, 5 December 2014 (UTC)[reply]

Is it necessary for the Wikipedia to flash the gory details of a formula?[edit]

The details of Köhn and Ebert result seem out of place in an article directed at general reader.


Full agree. Wikipedia is not the place to develop such complex formula that 99.9% of readers cannot even udnerstand. It is by far more useful to place it in this talk.

Here is the development of the Formula for experts:

with

This expression can be derived by using a quantum mechanical symmetry between pair production and Bremsstrahlung.
is the atomic number, the fine structure constant, the reduced Planck's constant and the speed of light. The kinetic energies of the positron and electron relate to their total energies and momenta via

Conservation of energy yields

The momentum of the virtual photon between incident photon and nucleus is:

where the directions are given via:

where is the momentum of the incident photon.

In order to analyse the relation between the photon energy and the emission angle between photon and positron, Köhn and Ebert integrated [1] the quadruply differential cross section over and . The double differential cross section is:

with

and

This cross section can be applied in Monte Carlo simulations.

References

  1. ^ Koehn, C., Ebert, U., Angular distribution of Bremsstrahlung photons and of positrons for calculations of terrestrial gamma-ray flashes and positron beams, Atmos. Res. (2013), http://dx.doi.org/10.1016/j.atmosres.2013.03.012

Revert regarding pair production in matter[edit]

This is a note explaning my revert of the edit that was just made. The paragraph beginning with this text is not about pair production in the vacuum:

In nuclear physics, this occurs when a high-energy photon interacts with an atomic nucleus, allowing it to decay into an electron and a positron without violating conservation of momentum. It is the chief method by which energy from gamma rays is observed in condensed matter.

It refers to a real photon decaying to an electron and a positron. Although there is no nuclear decay involved, a nucleus is required to conserve momentum. If that were not true, photons with E > 1.022 MeV would decay extremely rapidly while moving through space; instead, it happens only in matter. -- SCZenz 14:49, 13 September 2005 (UTC)[reply]

Info from anon that can be properly formatted and added[edit]

• Usually occurs near a nucleus (only a negligible amount of energy is transferred to the nucleus, but momentum is not conserved.).

• hν – 1.022 MeV = E+ + E-, that is the energy of the positron plus the energy of the electron is equal to the energy of the original photon minus the rest mass of the two created particles.

• The attenuation cooeficient is proportional to Z-squared, and has a logarithmic dependence on the photon energy

• Because the probability increases rapidly with energy above the threshold level (1.022MeV), higher energy megavoltage beams can, in fact, be less penetrating than lower energy beams, particularly in high Z materials.

• Nuclear attraction and repulsion tend to give the positron slightly more energy than the electron.

• If pair production occurs in the field of an electron, it is called Triplet Production: o Three particles appear, the original electron, the created electron and the created positron. o The threshold for triplet production is 2.04 MeV o Small probability compared to pair production (for Pb, Z = 82, triplet probability ~ 0.01 x pair probability.


• Significant compared to Compton effect when hν → 10 MeV and Z ≥ 10

• In radiotherapy, pair production can occur in bones, increasing the dose to bone.

Production of heavier particles[edit]

The photon need only have a total energy of twice the rest mass(me) of an electron (1.022 MeV) for this to occur as described above; if it is much more energetic, heavier particles may also be produced.

What are these "heavier particles"? - Quirk 09:03, 21 May 2007 (UTC)[reply]

Muons and tauons - it requires the photon to be more than twice the rest mass of these particles. Agger 09:12, 19 June 2007 (UTC)[reply]

Curiosity on photon-photon pair production[edit]

Article says: photon-photon pair production may occur at 511 KeV, comparing it to photon-nucleus pair production. This leaves me wondering how the photon-photon version might work: it means photons could as well interact with other photons to produce particle-antiparticle pairs? -- Alessandro Ghignola (talk) 09:07, 25 April 2010 (UTC)[reply]

P.S. Nevermind, I've found it here, but perhaps a link to that article may be given in the text. -- Alessandro Ghignola (talk) 09:19, 25 April 2010 (UTC)[reply]

A single photon cannot split into two photons without additional particles involved, since that would violate conservation of angular momentum. Photons have spin one, whereas two photons have a cumulative spin of either zero (1 − 1) or two (1 + 1). Theoretically, a spin-two graviton or a spin-zero higgson could produce photon pairs though. Nicole Sharp (talk) 17:05, 20 September 2016 (UTC)[reply]

Conservation of Momentum[edit]

Why couldn't the newly created positron and electron absorb the momentum of the photon? How would the conservation law break without a nucleus? The article doesn't give a reason for this, just states this as a fact. Could someone shed some light on this? PAStheLoD (talk) 02:54, 8 June 2010 (UTC)[reply]

Math[edit]

There is a significant chunk of math in this article, would it be wise to break it down some and explain it? I don't have a problem with pretty math, but since wikipedia likes for the common man to be able to understand things, we should probably do something to make the math more presentable to a wider audience. 76.198.38.250 (talk) 20:00, 20 July 2013 (UTC)[reply]

Feynman Diagram[edit]

The Feynman diagram does not conserve momentum, so the interaction shown is only possible for a virtual pair production (though the diagram shows free pair production). 76.181.69.229 (talk) 22:00, 2 December 2013 (UTC)[reply]

I hope this is just my computer going wrong[edit]

http://puu.sh/gMWBX/ac4241b70a.png Am I the only one that sees a huge space here? Even if I am not, it's odd that there's something that large on the page. Is it a formula that didn't load? (I refreshed.) — Preceding unsigned comment added by Mechanic1c (talkcontribs) 23:28, 23 March 2015 (UTC)[reply]

Z[edit]

I think we should relabel "Z" as "nucleus" instead in the diagram shown to avoid confusion with the Z boson of the weak interaction. See "commons:file talk:Pair production Cartoon.gif#Z." Nicole Sharp (talk) 17:08, 20 September 2016 (UTC)[reply]

Basic Kinematics section has some serious mistakes[edit]

There are some serious mistakes in the section on Basic Kinematics. The conclusion is that the electron and positron are produced back-to-back. This is clearly wrong. As anyone who has seen photons convert to e+e- in bubble chamber photographs, they are produced with an almost zero opening angle not 180 degrees.

The problem with the maths is easy to see. (1+cos(theta)) is really (1-cos(theta)). Tracing this back, the minus sign follows from "E"-"p" not "E"+"p" which is the Minkowski geometry of spacetime.

So this section needs to be re-done, preferably with some better explanations of the approximations being used. For example, the statement that the nucleus has negligible mass compared to the energy of the photon would only be true for photon energies above several hundred GeV.

Chris Bowdery — Preceding unsigned comment added by 2A02:C7D:541A:1400:C595:135F:3FF6:64F3 (talk) 21:23, 23 October 2016 (UTC)[reply]

Photon is not an elementary particle[edit]

Looking at the first sentences, I see an error - "Pair production is the creation of an elementary particle and its antiparticle. Examples include creating an electron and a positron, a muon and an antimuon, or a proton and an antiproton" - if it is the creation of an elementary particle and its antiparticle then a proton and an antiproton, which are composed of quarks/antiquarks, would not qualify. This needs to be clarified. --Nerd1a4i (talk) 13:02, 15 July 2017 (UTC)[reply]

Basic kinematics - Energy and momentum conservation[edit]

The section "Basic kinematics" is inaccurate. Specifically, according to the metric signature (−, +, +, +) and with the assumption that the modulus of the velocity of the electron and the positron is the same, and that is the angle between the two velocity vectors (as in the article), the calculation gives

and hence

The equality can be true only if and , that is clearly impossible for electrons and positrons. The underlying reason is that the equality holds for massless particles like photons, but not for massive particles like electrons and positrons, unless they move at the velocity of light (that is impossible for massive particles). Therefore, it is not possible to assure energy and momentum conservation when a single photon decays in massive particles without the interaction with other particles. Szunino81 (talk) 13:19, 7 September 2017 (UTC)[reply]

Hawking radiation is not pair production by the definition given here[edit]

The article mentions Hawking radiation (under the heading "Astronomy", which incidentally is ridiculous), but Hawking radiation does not involve a neutral boson. More generally, there are lots of other forms of pair production that also do not involve a neutral boson - Schwinger pair production, pair production in plasma, pair production from the collision of two (high energy) photons, etc. So, either the lede should be rewritten to include these other phenomena, or it should make clear that it is not discussing them and the reference to Hawking radiation should be deleted. I think the first option is better. Waleswatcher (talk) 21:26, 18 April 2018 (UTC)[reply]

History[edit]

This article could use a bit of history. I'd imagine the first observation of pair production was quite notable and surprising, but it's not mentioned at all. — Preceding unsigned comment added by 96.40.48.159 (talk) 14:05, 29 June 2018 (UTC)[reply]

About the conservation of momentum and energy[edit]

The photon must be near a nucleus in order to satisfy conservation of momentum, as an electron–positron pair produced in free space cannot satisfy conservation of both energy and momentum.

Actually it does not require a nucleus. It requires a second particle.

The problem is the free choice of the reference frame. The energy of the photon depends on the frame of reference. It can have any positive value, see Relativistic_Doppler_effect.

So we have an initial state, where we have only one photon with an arbitrary energy, depending on our choice of reference frame. In the final state however we have two particles. These particles have rest mass, and so the total energy in the final state must be at least equal to the rest masses of the produced particles. This contradicts the free choice of the reference frame, and thus impossible.

I believe there is another explanation involving Feynman diagrams. There are rules for drawing Feynman diagrams, and there can not be a process where only one particle enters the diagram and more particles leave.

However these are both indirect explanations. Cs.B. (talk) 19:36, 1 February 2023 (UTC)[reply]

Minimum energy required[edit]

As energy must be conserved, for pair production to occur, the incoming energy of the photon must be above a threshold of at least the total rest mass energy of the two particles created. (As the electron is the lightest, hence, lowest mass/energy, elementary particle, it requires the least energetic photons of all possible pair-production processes.)

The explanation is not factually correct, since the electron is not the lightest particle. Neutrinos are lighter. I can not provide explanation on why neutrino-antineutrino pair production does not occur (or does it?). It may be related to the interactions, since photons are only known to interact via electromagnetism and gravity, where neutrinos do not interact with electromagnetism. Maybe there is neutrino-antineutrino pair production involving other bosons.

Cs.B. (talk) 19:44, 1 February 2023 (UTC)[reply]